| NGC 5011 | |
|---|---|
 HST image of NGC 5011B (right) and NGC 5011C (left) | |
| Observation data (J2000 epoch) | |
| Constellation | Centaurus |
| Right ascension | 13h 12m 51.848s[1] |
| Declination | −43° 05′ 46.25″[1] |
| Redshift | 0.010537[2] |
| Heliocentric radial velocity | 3159 km/s[2] |
| Distance | 133.26 ± 18.56 Mly (40.857 ± 5.692 Mpc)[2] |
| Apparent magnitude (V) | 11.33[3] |
| Apparent magnitude (B) | 12.14[3] |
| Characteristics | |
| Type | E1-2[2] |
| Size | 92,800 ly (28,440 pc)[2][note 1] |
| Apparent size (V) | 1.763′ × 1.552′[1][note 1] |
| Other designations | |
| MGC-07-27-042, PGC 45898[3] | |
NGC 5011 is an elliptical galaxy in the constellation of Centaurus.[2] It was discovered on 3 June 1834 by John Herschel.[4] It was described as "pretty bright, considerably small, round, among 4 stars" by John Louis Emil Dreyer, the compiler of the New General Catalogue.[4]
- ^ a b c Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- ^ a b c d e f "NED results for object NGC 5011". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 6 September 2017.
- ^ a b c "NGC 5011". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 6 September 2017.
- ^ a b "New General Catalog Objects: NGC 5000 - 5059". cseligman.com. Retrieved 6 September 2017.
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